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Dynamics of Multiple Stellar Populations in Globular Clusters

Published online by Cambridge University Press:  05 March 2015

Enrico Vesperini ,
Steve McMillan ,
Franca D'Antona  and
Annibale D'Ercole
Enrico Vesperini
Affiliation:
Department of Astronomy, Indiana University, Bloomington, IN 47401, USA
Steve McMillan
Affiliation:
Department of Physics, Drexel University, Philadelphia, PA, 19104, USA
Franca D'Antona
Affiliation:
INAF- Osservatorio Astronomico di Roma, via di Frascati 33, I-00040 Monteporzio, Italy
Annibale D'Ercole
Affiliation:
INAF- Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, Italy
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Abstract

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The results of numerous spectroscopic and photometric studies have revealed the presence of multiple stellar populations in many globular clusters. In this paper we summarize the results of our recent studies on the dynamical evolution of multiple-population clusters, the implications of the structural properties of multiple-population clusters for the evolution of binary stars, and the possible contribution of globular clusters to the assembly of the Galactic halo.

Keywords

(Galaxy:) globular clusters: generalstellar dynamicsmethods: n-body simulations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 251 - 252
Copyright
Copyright © International Astronomical Union 2015 

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